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Cited article:

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Dust–gas dynamics driven by the streaming instability with various pressure gradients

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Streaming Instability and Turbulence: Conditions for Planetesimal Formation

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Dust Coagulation Reconciles Protoplanetary Disk Observations with the Vertical Shear Instability. I. Dust Coagulation and the VSI Dead Zone

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Formation of the First Planetesimals via the Streaming Instability in Globally Turbulent Protoplanetary Disks?

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